Interstellar dust; Contributed papers
Conference
·
OSTI ID:6257545
A coherent picture of the dust composition and its physical characteristics in the various phases of the interstellar medium was the central theme. Topics addressed included: dust in diffuse interstellar medium; overidentified infrared emission features; dust in dense clouds; dust in galaxies; optical properties of dust grains; interstellar dust models; interstellar dust and the solar system; dust formation and destruction; UV, visible, and IR observations of interstellar extinction; and quantum-statistical calculations of IR emission from highly vibrationally excited polycyclic aromatic hydrocarbon (PAH) molecules.
- Research Organization:
- National Aeronautics and Space Administration, Moffett Field, CA (USA). Ames Research Center
- OSTI ID:
- 6257545
- Report Number(s):
- N-91-14897; NASA-CP--3036; A--89050; NAS--1.55:3036; CONF-8807213--
- Country of Publication:
- United States
- Language:
- English
Similar Records
VERY LARGE INTERSTELLAR GRAINS AS EVIDENCED BY THE MID-INFRARED EXTINCTION
Interstellar polycyclic aromatic hydrocarbons - The infrared emission bands, the excitation/emission mechanism, and the astrophysical implications
Composition, structure and chemistry of interstellar dust
Journal Article
·
Sun Sep 20 00:00:00 EDT 2015
· Astrophysical Journal
·
OSTI ID:22525419
Interstellar polycyclic aromatic hydrocarbons - The infrared emission bands, the excitation/emission mechanism, and the astrophysical implications
Journal Article
·
Thu Nov 30 23:00:00 EST 1989
· Astrophysical Journal, Supplement Series; (USA)
·
OSTI ID:6966798
Composition, structure and chemistry of interstellar dust
Technical Report
·
Mon Sep 01 00:00:00 EDT 1986
·
OSTI ID:5554510